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By Bernard Guinot (auth.), Heinrich K. Eichhorn, Robert J. Leacock (eds.)
Read Online or Download Astrometric Techniques: Proceedings of the 109th Symposium of the International Astronomical Union Held in Gainesville, Florida, U.S.A., 9–12 January 1984 PDF
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Extra resources for Astrometric Techniques: Proceedings of the 109th Symposium of the International Astronomical Union Held in Gainesville, Florida, U.S.A., 9–12 January 1984
Astrometric Techniques, 43-45. 1986 by the [AU. HANSON Hanson (1983) has devised a powerful new method to use the distribution N(H) of reduced proper motions to determine the stellar luminosity function. , (1) taking the slope 6M/6H as a free parameter in determining M from H, (2) implicitly equating C(MIH) with C(HIM)]. Moreover, the new method allows more reliance on empirical tests than on kinematical assumptions, and dispen~es with the trigonometric parallax calibrations, incompleteness corrections, and distance limits needed in other luminosity function determinations.
R. ) + A . R. + B .. (R. ) + B . -1 -1 -] 0] -] 1] -] 0] R. ]• -] (9) Substituting zero as the value of all planetary masses into the relativistic right-hand members of Eq. (9) leads to the Schwarzschild terms. Relativistic perturbations in the motion of the major planets have been investigated in detail by Lestrade and Bretagnon (1982). With the aid of Eq. (8) applied to the three body problem: Earth, Sun and Moon one may derive the relativistic equations of the Lunar motion in the form adapted for numerical integration (Brumberg and Ivanova 1982).
Proc. Symp. 5 lAG, 26. S. 1979. Lorentzian Basis and Gravitational Effects in the Einsteinian Theory of Gravitation. Minsk (in Russian). N. 1982. -mat. 5, 84. L. S. 1981. Doklady AN USSR 261, 1320. F. and Bretagnon P. 1982. Astron. Astrophys. 105, 42. F. and Chapront-Touze' M. 1982. Astron. Astrophys. 116, 75. K. W. 1963. J. Math. Phys. 4, 735. B. and Strathdee J. 1959. Proc. R. Soc. A252, 476. 42 V. A. BRUMBERG Mikhailov A•. 1969. Astron. Zh. (USSR) 46, 454. M611er C. 1972. The Theory of Relativity.